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Astrophysics Gallery

Available as Prints and Gift Items

Choose from 933 pictures in our Astrophysics collection for your Wall Art or Photo Gift. All professionally made for Quick Shipping.


Pale Blue Dot, Voyager 1
Pale Blue Dot, Voyager 1
Science Photo Library

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Hubble Ultra Deep Field 2012
Hubble Ultra Deep Field 2012
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MAP microwave background
MAP microwave background
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1919 solar eclipse
1919 solar eclipse
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1919 solar eclipse
1919 solar eclipse
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Orion nebula
Orion nebula
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Pillars of Creation
Pillars of Creation
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Nebula Sh 2-106, HST image
Nebula Sh 2-106, HST image
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Gas pillars in the Eagle Nebula
Gas pillars in the Eagle Nebula
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Hubble Ultra Deep Field galaxies
Hubble Ultra Deep Field galaxies
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Cosmic microwave background
Cosmic microwave background
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Orions belt
Orions belt
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Pale Blue Dot, Voyager 1 Featured Image

Pale Blue Dot, Voyager 1

This unique narrow-angle color image is of the Earth, dubbed Pale Blue Dot, is a part of the first ever portrait of the solar system taken by Voyager 1. The spacecraft acquired a total of 60 frames for a mosaic of the solar system from a distance of more than 4 billion miles from Earth and about 32 degrees above the ecliptic. From Voyager's great distance Earth is a mere point of light, less than the size of a picture element even in the narrow-angle camera. Earth was a crescent only 0.12 pixel in size. Coincidentally, Earth lies right in the center of one of the scattered light rays resulting from taking the image so close to the sun. This blown-up image of the Earth was taken through three color filters -- violet, blue and green -- and recombined to produce the color image. The background features in the image are artifacts resulting from the magnification

© NASA/SCIENCE PHOTO LIBRARY

Sombrero galaxy (M104), HST image
Sombrero galaxy (M104), HST image
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Milky Way
Milky Way
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Antennae colliding galaxies, Hubble image
Antennae colliding galaxies, Hubble image
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Crab nebula (M1)
Crab nebula (M1)
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Orion nebula (M42)
Orion nebula (M42)
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Hale-Bopp comet
Hale-Bopp comet
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Eagle Nebula
Eagle Nebula
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Diagram showing the spectral class and luminosity of stars
Diagram showing the spectral class and luminosity of stars
Stocktrek Images

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Solar system
Solar system
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Supernova in galaxy
Supernova in galaxy
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Crab nebula, composite image
Crab nebula, composite image
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Moon rising over Earths horizon
Moon rising over Earths horizon
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Diagram showing the spectral class and luminosity of stars Featured Image

Diagram showing the spectral class and luminosity of stars

Diagram showing the spectral class and luminosity of stars. The diagram was named The Hertzsprung-Russell Diagram, or the H-R diagram for short. At the beginning of the 20th century two astronomers found that if stars were plotted on a diagram with their luminosity (brightness) on one axis, and their spectral class on the other, that stars formed three distinct groups. The largest group, the Main Sequence Stars, is where 90% of the stars are found. These stars are fusing hydrogen into helium in their cores. This group propagates diagonally from the upper left corner, down to the right corner. The group below the main sequence is the White Dwarfs, which is a group of small, earth-sized stellar remnants. The third group, which is found above the main sequence is that of the giants.
Stars appear on a specific place on the main sequence depending on their mass and age. The mass determines when it will leave the main sequence.The H-R diagram is a significant tool for astronomers, when it comes to understanding stellar evolution

© Fahad Sulehria/Stocktrek Images

A galactic light show in spiral galaxy NGC 4258
A galactic light show in spiral galaxy NGC 4258
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Light echoes from exploding star
Light echoes from exploding star
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Supernova explosion, artwork
Supernova explosion, artwork
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Aurora over Antarctica, satellite image
Aurora over Antarctica, satellite image
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Saturn, Cassini image
Saturn, Cassini image
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Solar System, artwork
Solar System, artwork
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The Orion Nebula
The Orion Nebula
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Horsehead Nebula
Horsehead Nebula
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Interacting galaxies NGC 5257 and 5258
Interacting galaxies NGC 5257 and 5258
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Helix nebula, infrared Spitzer image
Helix nebula, infrared Spitzer image
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Planetary nebula
Planetary nebula
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Mars, composite satellite images
Mars, composite satellite images
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Helix nebula, infrared Spitzer image Featured Image

Helix nebula, infrared Spitzer image

Helix nebula (NGC 7293), infrared Spitzer Space Telescope image. This is a planetary nebula, a series of shells of gas cast off by a dying star. The ejection of the star's outer layers exposes its hot core, whose radiation ionises the shells, causing them to glow. This image was taken at wavelengths of varying energy: high (blue), medium (green) and low (red). The gas in the central regions has been ionised more than the outer gas, which is shielded from the stellar core. The most highly ionised areas (cometary heads) are round the edge of the central void. Foreground and background stars are blue. The Helix nebula is 650 light years from Earth, in the constellation of Aquarius. Image data obtained by the IRAC sensor in October 2004

© NASA/JPL-CALTECH/J. HORA (HARVARD-SMITHSONIAN CfA)/SCIENCE PHOTO LIBRARY

Spiral galaxy M81, composite image
Spiral galaxy M81, composite image
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Kepler Mission space telescope, artwork
Kepler Mission space telescope, artwork
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Orbit of Sputnik 1, Soviet 1957 diagram
Orbit of Sputnik 1, Soviet 1957 diagram
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Interacting galaxies Arp 147, HST image
Interacting galaxies Arp 147, HST image
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Io and Jupiter, Cassini image
Io and Jupiter, Cassini image
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Ring Nebula M57, Hubble image C017/3725
Ring Nebula M57, Hubble image C017/3725
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Edwin Hubble, US astronomer C008/8831
Edwin Hubble, US astronomer C008/8831
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Interacting galaxies
Interacting galaxies
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Cigar galaxy (M82), composite image
Cigar galaxy (M82), composite image
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Milky Way
Milky Way
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Dark matter distribution
Dark matter distribution
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Orion nebula (M42 and M43)
Orion nebula (M42 and M43)
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